Category Archives: Phys.org
En route to Jupiter, Europa Clipper captures images of stars
Interaction of kinetic waves and suprathermal particles could be key to unlocking biggest mystery in heliophysics

A graduate research assistant at The University of Alabama in Huntsville (UAH), a part of The University of Alabama system, has published a paper in the journal Astronomy & Astrophysics that builds on an earlier study to help understand why the solar corona is so hot compared to the surface of the sun itself.
Burrowing mole-bot could characterize other planets’ soil
High-precision spectrograph confirms massive exoplanet orbiting a low-mass star

With an assist from the NEID spectrograph, a team of astronomers have confirmed the existence of exoplanet Gaia-4b—one of the most massive planets known to orbit a low-mass star. Gaia-4b is also the first planet detected by the European Space Agency’s Gaia spacecraft using the astrometric technique.
Trench-like features on Uranus’s moon Ariel may be windows to its interior

Last year, a study led by planetary scientist Richard Cartwright at the Johns Hopkins Applied Physics Laboratory (APL) in Laurel, Maryland, proposed that deposits of carbon dioxide ice and other carbon-bearing molecules on Uranus’s moon Ariel likely originated from chemical processes inside the moon—possibly even from a subsurface ocean.
Webb investigates dusty and dynamic protoplanetary disk HH 30
Lunar rocks help scientists pinpoint when the moon crystallized
SETI researchers double-check 1 million objects for signs of alien signals

We can’t help ourselves but wonder about life elsewhere in the universe. Any hint of a biosignature or even a faint, technosignature-like event wrests our attention away from our tumultuous daily affairs. In 1984, our wistful quest took concrete form as SETI, the Search for Extraterrestrial Intelligence.
JWST unveils the mysteries of distant quiescent galaxies: Why do they stop growing?

Galaxies are astronomical objects composed of billions or even trillions of stars. Our Earth and solar system are just a tiny part of the Milky Way; it is one of countless galaxies in the universe. These immense systems are the fundamental building blocks of cosmic structure. During the universe’s 13.7 billion-year history, the first few billion years marked a golden age for galaxy formation, when galaxies actively turned their gas reservoirs into new stars.
Collaboration uncovers how gravity influences qubits
Boeing Starliner official talks pros and cons of NASA contracts
SpaceX pushes Kennedy Space Center launch to Tuesday, could bring sonic boom with booster landing
Quantum machine simulates universe’s potential false vacuum decay
Mount Rainier white-tailed ptarmigan finally receives a ‘threatened’ species designation
Six things to know about SPHEREx, NASA’s newest space telescope
NASA radar imagery reveals details about Los Angeles–area landslides
Can ocean-floor mining oversights help regulate space debris and mining on the moon?
Hubble captures supernova-hosting galaxy in the constellation Gemini

The subject of this NASA/ESA Hubble Space Telescope image is a supernova-hosting galaxy located about 600 million light-years away in the constellation Gemini. Hubble captured this image roughly two months after a supernova named SN 2022aajn was discovered. The supernova is visible as a blue dot at the center of the image, brightening the hazy body of the galaxy.
Measuring light sail performance in the lab

Sailing has been a mainstay of human history for millennia, so it’s no surprise that scientists would apply it to traveling in space. Solar sailing, the most common version, uses pressure from the sun to push spacecraft with giant sails outward in the solar system. However, there is a more technologically advanced version that several groups think might offer us the best shot at getting to Alpha Centauri—light sailing.